Speaker
Sanja Danilovic
(Max Planck Institute for Solar System Research)
Description
Recent SST observations have given a new definition of Ellerman bombs (EBs). They are
short-lived flame-like features visible in the wings of Halpha, away from the disc
center. EBs seem to be associated with a peculiar combination of signatures in
different observables. Also, they could be placed on, energetically, a low end of the
whole spectrum of events that might have the same physical process triggering them.
Can we simulate them? How are they formed? What field configuration produces them? We
address these issues by using MURaM simulations.
Primary author
Sanja Danilovic
(Max Planck Institute for Solar System Research)
